Genesis of Flux Ropes Observed by Pioneer-Venus Orbiter in the Photoequilibrium Region At Venus

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dc.creatorKrymskii, A. M.
dc.creatorBojkov, D. I.
dc.date1998-12-29
dc.date.accessioned2026-07-07T02:29:50Z
dc.date.available2026-07-07T02:29:50Z
dc.descriptionGenesis of flux ropes observed by Pioneer-Venus Orbiter in the photoequilibrium region at Venus is analysed. Stability analysis of the large-scale magnetic field pushed deep inside during period of high dynamic pressure of solar wind had shown that the top-side boundary of the magnetic belt located within the region of photoequilibrium is unstable. The finite conductivity of plasma tends to stabilise the instability so that the bottom-side part of the magnetic belt is regular. Non-numerous flux ropes which were observed above the predicted instability region are likely moving upward because of the magnetic buoyancy.
dc.descriptionHTML format, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/9812461
dc.identifierhttp://arxiv.org/abs/astro-ph/9812461
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13627
dc.subjectAstrophysics
dc.titleGenesis of Flux Ropes Observed by Pioneer-Venus Orbiter in the Photoequilibrium Region At Venus
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